|15:00 UT||17:00 UT||19:03 UT||21:00 UT|
|23:00 UT||01:03 UT||03:00 UT||05:00 UT|
Click on the thumbnails for 256 x 256 pixel, full-resolution GIF images.
The dark lane is narrowing by 1996 November 29 01:03 UT, and is beginning to fill in by 05:00 UT.
Sorry we don't have more frequent images, but (as of this writing), EIT has very limited telemetry for anything besides a very sparse synoptic, which includes Fe XII 195 Å images such as these obtained every 2 hours. Because of the bandwidth limitation, all but one of these per day is binned 2 x 2 on the detector.
Note that the low-lying aracde of loops that form below and after the CME-swept dark lane is similar to that in the much better observed (by EIT, at least) CME of 1996 November 30 - December 1, apparently from the same filament channel --- the same filament channel that has been producing most of the big CME's since 1996 July.
Last revised - J.B. Gurman